A correlation-locking adaptive filtering technique for minimum variance integral control in adaptive optics
| dc.contributor.author | Deo, V | |
| dc.contributor.author | Gendron, Eric | |
| dc.contributor.author | Vidal, Fabrice | |
| dc.contributor.author | Rozel, M | |
| dc.contributor.author | Sevin, A | |
| dc.contributor.author | Ferreira, F | |
| dc.contributor.author | Gratadour, Damien | |
| dc.contributor.author | Galland, N | |
| dc.contributor.author | Rousset, Gerard | |
| dc.date.accessioned | 2023-03-06T21:35:32Z | |
| dc.date.available | 2023-03-06T21:35:32Z | |
| dc.date.issued | 2021 | |
| dc.date.updated | 2021-12-26T07:18:35Z | |
| dc.description.abstract | We propose the correlation-locking optimization scheme (CLOSE), a real-time adaptive filtering technique for adaptive optics (AO) systems controlled with integrators. CLOSE leverages the temporal autocorrelation of modal signals in the controller telemetry and drives the gains of the integral command law in a closed servo-loop. This supervisory loop is configured using only a few scalar parameters and automatically controls the modal gains to closely match transfer functions achieving minimum variance control. This optimization is proven to work throughout the range of noise and seeing conditions relevant to the AO system. This technique was designed while preparing the high-order AO systems for extremely large telescopes, in particular to tackle the optical gain (OG) phenomenon. This is a sensitivity reduction induced by on-sky residuals and is a prominent issue with pyramid wavefront sensors (PWFS). CLOSE follows upon the linear modal compensation approach to OG that was previously demonstrated to substantially improve AO correction with high-order PWFS systems. Operating on modal gains through multiplicative increments, CLOSE naturally compensates for the recurring issue of unaccounted sensitivity factors throughout the AO loop. We present end-to-end simulations of the MICADO instrument single-conjugate AO to demonstrate the performances and capabilities of CLOSE. We demonstrate that a single configuration provides an efficient and versatile optimization of the modal integrator while accounting for OG compensation and while providing significant robustness to transient effects impacting the PWFS sensitivity. | en_AU |
| dc.description.sponsorship | This research is performed in the frame of the development of MICADO, first light instrument of the ELT (ESO), with the support of ESO, INSU/CNRS and Observatoire de Paris. V. Deo is supported by NASA grant 80NSSC19K0336. Additional support was provided through the WOLF project, ANR-18-CE31-0018 of the French National Research Agency (ANR), and the OPTICON Program of the European Commission (H2020, Grant number 730890). The authors thank the COMPASS development and support team for their continued support. | en_AU |
| dc.format.mimetype | application/pdf | en_AU |
| dc.identifier.issn | 0004-6361 | en_AU |
| dc.identifier.uri | http://hdl.handle.net/1885/286647 | |
| dc.language.iso | en_AU | en_AU |
| dc.provenance | Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. | en_AU |
| dc.publisher | Springer | en_AU |
| dc.rights | © 2021 The authors | en_AU |
| dc.rights.license | Creative Commons Attribution licence | en_AU |
| dc.rights.uri | http://creativecommons.org/licenses/by/4.0/ | en_AU |
| dc.source | Astronomy and Astrophysics | en_AU |
| dc.subject | instrumentation: adaptive optics | en_AU |
| dc.subject | techniques: high angular resolution | en_AU |
| dc.subject | telescopes | en_AU |
| dc.title | A correlation-locking adaptive filtering technique for minimum variance integral control in adaptive optics | en_AU |
| dc.type | Journal article | en_AU |
| dcterms.accessRights | Open Access | en_AU |
| local.contributor.affiliation | Deo, V, Sorbonne Universite | en_AU |
| local.contributor.affiliation | Gendron, Eric, CNRS-Universite Paris Diderot | en_AU |
| local.contributor.affiliation | Vidal, Fabrice, CNRS-Universite Paris Diderot | en_AU |
| local.contributor.affiliation | Rozel, M, Sorbonne Universite | en_AU |
| local.contributor.affiliation | Sevin, A, Sorbonne Universite | en_AU |
| local.contributor.affiliation | Ferreira, F, Sorbonne Universite | en_AU |
| local.contributor.affiliation | Gratadour, Damien, College of Science, ANU | en_AU |
| local.contributor.affiliation | Galland, N, Sorbonne Universite | en_AU |
| local.contributor.affiliation | Rousset, Gerard, Observatoire de Paris | en_AU |
| local.contributor.authoruid | Gratadour, Damien, u1079122 | en_AU |
| local.description.notes | Imported from ARIES | en_AU |
| local.identifier.absfor | 510102 - Astronomical instrumentation | en_AU |
| local.identifier.absfor | 510203 - Nonlinear optics and spectroscopy | en_AU |
| local.identifier.absfor | 400909 - Photonic and electro-optical devices, sensors and systems (excl. communications) | en_AU |
| local.identifier.absseo | 280120 - Expanding knowledge in the physical sciences | en_AU |
| local.identifier.absseo | 280110 - Expanding knowledge in engineering | en_AU |
| local.identifier.ariespublication | a383154xPUB19732 | en_AU |
| local.identifier.citationvolume | 650 | en_AU |
| local.identifier.doi | 10.1051/0004-6361/202040216 | en_AU |
| local.identifier.scopusID | 2-s2.0-85107613089 | |
| local.publisher.url | https://www.aanda.org/ | en_AU |
| local.type.status | Published Version | en_AU |
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